Table 12: Probable late-type cluster members based on proper motion (Platais et al. 2001) that were not detected in X-rays.
Platais# V B-V log $L_{\rm x}$ log $\frac{L_{\rm x}}{L_{\rm bol}}$ Notes

987 13.51 1.12 <28.55 <-4.33

1238 12.75 0.68 - <-4.63 *

1315 12.30 0.81 <28.95 <-4.27

1574 14.13 1.17 <29.11 <-3.57

2223 11.04 0.59 <28.53 <-5.15

2767 12.11 0.95 <28.76 <-4.59

3678 11.49 0.67 <28.50 <-5.01

6567 13.46 1.23 *

6783 14.17 0.67 - <-3.74 *

6819 13.42 0.88 - <-4.48 *

8409 13.39 1.06 <28.83 <-4.09

8422 13.04 1.01 <29.08 <-3.92

Notes:
#1238: photometry suggests membership of cluster B.
#6567: no X-ray upper limit because too close to X177.
#6783: photometry suggests non-membership.
#6819: photometry suggests membership of cluster B.

**Table 12:** Probable late-type cluster members based on proper motion (Platais et al. 2001) that were not detected in X-rays.
Platais#	V	B-V	log $L_{\rm x}$	log $\frac{L_{\rm x}}{L_{\rm bol}}$	Notes
987	13.51	1.12	<28.55	<-4.33
1238	12.75	0.68	-	<-4.63	*
1315	12.30	0.81	<28.95	<-4.27
1574	14.13	1.17	<29.11	<-3.57
2223	11.04	0.59	<28.53	<-5.15
2767	12.11	0.95	<28.76	<-4.59
3678	11.49	0.67	<28.50	<-5.01
6567	13.46	1.23			*
6783	14.17	0.67	-	<-3.74	*
6819	13.42	0.88	-	<-4.48	*
8409	13.39	1.06	<28.83	<-4.09
8422	13.04	1.01	<29.08	<-3.92

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